Английская Википедия:1573 Väisälä

Материал из Онлайн справочника
Перейти к навигацииПерейти к поиску

Шаблон:Short description Шаблон:Infobox planet

1573 Väisälä, provisional designation Шаблон:Mp, is a stony Phocaea asteroid, slow rotator and suspected tumbler from the inner regions of the asteroid belt, approximately 9 kilometers in diameter. It was discovered on 27 October 1949, by Belgian astronomer Sylvain Arend at the Royal Observatory of Belgium in Uccle, Belgium.[1] It was named for Finnish astronomer Yrjö Väisälä.[2]

Orbit and classification

The stony S-type asteroid is a member of the Phocaea family (Шаблон:Small), a group of asteroids with similar orbital characteristics.[3] It orbits the Sun at a distance of 1.8–2.9 AU once every 3 years and 8 months (1,334 days). Its orbit has an eccentricity of 0.23 and an inclination of 25° with respect to the ecliptic.[4] VäisäläШаблон:'s observation arc begins on the night following its official discovery observation at Uccle, as no precoveries were taken and no prior identifications were made.[1]

Physical characteristics

Slow rotator

In September 2011, a rotational lightcurve of Väisälä was obtained from photometric observations made by Czech astronomer Petr Pravec at Ondřejov Observatory.Шаблон:Efn Its analysis gave a rotation period of 252 hours with a brightness variation of 0.76 magnitude (Шаблон:Small).Шаблон:Efn This makes Väisälä one of the Top 200 slow rotators known to exist. The body is also suspected to be in a non-principal axis rotation (NPAR), colloquially called as "tumbling". As of 2017, no follow-up observations have been made of these provisional results.[5]

Diameter and albedo

According to the space-based surveys carried out by the Infrared Astronomical Satellite IRAS, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Väisälä measures between 8.43 and 9.77 kilometers in diameter, and its surface has an albedo between 0.222 and 0.284.[6][7][8][9] The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.2226 and a diameter of 9.77 kilometers using on an absolute magnitude of 12.30.[5]

Naming

This minor planet was named after Finnish astronomer, Yrjö Väisälä (1891–1971), a prolific discoverer of minor planets during the late 1930s and early 1940s.[2] In addition, a second minor planet, 2804 Yrjö, was named in his honor by pioneering Finnish female astronomer Liisi Oterma, and the lunar crater Väisälä also bears his name. The official Шаблон:MoMP was published by the Minor Planet Center on 31 January 1962 (Шаблон:Small).[10]

Notets

Шаблон:Notelist

References

Шаблон:Reflist

External links

Шаблон:Use dmy dates Шаблон:Minor planets navigator Шаблон:Small Solar System bodies

  1. 1,0 1,1 Ошибка цитирования Неверный тег <ref>; для сносок MPC-Vaisala не указан текст
  2. 2,0 2,1 Ошибка цитирования Неверный тег <ref>; для сносок springer не указан текст
  3. Ошибка цитирования Неверный тег <ref>; для сносок Ferret не указан текст
  4. Ошибка цитирования Неверный тег <ref>; для сносок jpldata не указан текст
  5. 5,0 5,1 Ошибка цитирования Неверный тег <ref>; для сносок lcdb не указан текст
  6. Ошибка цитирования Неверный тег <ref>; для сносок Nugent-2016 не указан текст
  7. Ошибка цитирования Неверный тег <ref>; для сносок WISE не указан текст
  8. Ошибка цитирования Неверный тег <ref>; для сносок Masiero-2011 не указан текст
  9. Ошибка цитирования Неверный тег <ref>; для сносок SIMPS не указан текст
  10. Ошибка цитирования Неверный тег <ref>; для сносок DoMP-Circular-dates не указан текст